Unravelling the Neoproterozoic Accretionary History of Oman, Using an Array of Isotopic Systems in Zircon.

The Omani basement is a critical window into the Neoproterozoic tectonic geography of the Mozambique Ocean and the amalgamation of Gondwana. It is located east of the juvenile arc terranes of the Arabian Nubian Shield (ANS), yet the relationship between the two is not well understood. Magmatic and detrital zircon samples were analysed from four main basement terranes; Mirbat, the Huqf, Jebel Ja9Alan and Al Jobah. The U–Pb (zircon) ages from igneous samples give ages between 838–765 Ma. The Lu–Hf and oxygen isotopes show that the zircons are juvenile (ɛHf(t) values 10.5–8.7), with low δ18O values (∼2–6‰). Detritus from sediments in Mirbat, the southern-most basement outcrop, preserves a main age peak at ca. 786 Ma, with Lu–Hf between +6.05 and +12.64, respectively. Lu–Hf isotopic data for Proterozoic detrital zircons from Jebel Ja9Alan suggest that this region was depositionally connected to a source yielding both evolved Tonian and Neoarchean to Palaeoproterozoic detritus. These sources could correlate to the terranes in India and South China, which record the similarly low δ18O values. These data support a model in which Oman formed in its own tectonic domain, accreting onto the Neoproterozoic active margin of a continent. Supplementary material: All U–Pb, hafnium and oxygen data have been included in the tables (1, 2 and 3 and 4 respectively). Figures including all weighted average plots (Fig 1) and Initial 176Hf/177Hf versus 206Pb/238U age (Fig. 2) are also included in the supplementary material to aid in identifying Pb-loss in the data. https://doi.org/10.6084/m9.figshare.c.4682363